Timeline for How protons come near to during the formation of a nucleus?
Current License: CC BY-SA 3.0
11 events
| when toggle format | what | by | license | comment | |
|---|---|---|---|---|---|
| Oct 29, 2016 at 4:27 | vote | accept | Saujatya Kole | ||
| Oct 29, 2016 at 4:25 | vote | accept | Saujatya Kole | ||
| Oct 29, 2016 at 4:27 | |||||
| Oct 29, 2016 at 4:25 | vote | accept | Saujatya Kole | ||
| Oct 29, 2016 at 4:25 | |||||
| Oct 28, 2016 at 20:27 | answer | added | Charlie | timeline score: 1 | |
| Oct 27, 2016 at 18:34 | history | edited | Qmechanic♦ |
edited tags
|
|
| Oct 27, 2016 at 17:29 | answer | added | freecharly | timeline score: 3 | |
| Oct 27, 2016 at 17:24 | comment | added | Gert | Two protons ('diproton') isn't actually a stable arrangement. But fusion of other proton containing nuclei can be achieved (e.g.) in the interior of stars, where the core temperature is near a billion Kelvin. In these conditions, the nuclei have such high kinetic energy that the work needed to overcome the electrostatic repulsion can be done. Once close enough together the short-range nuclear forces do the 'binding' of the nuclei. | |
| S Oct 27, 2016 at 17:10 | history | suggested | Spoilt Milk | CC BY-SA 3.0 |
Checked grammar, corrected spelling
|
| Oct 27, 2016 at 17:06 | review | First posts | |||
| Oct 27, 2016 at 18:53 | |||||
| Oct 27, 2016 at 17:06 | review | Suggested edits | |||
| S Oct 27, 2016 at 17:10 | |||||
| Oct 27, 2016 at 17:03 | history | asked | Saujatya Kole | CC BY-SA 3.0 |